Existing Rossiter-McLaughlin measurements of wide-orbiting planets suggest that this population may have an intrinsically different spin-orbit angle distribution from the shorter-period hot Jupiter population. In particular, the trend of systematically lower obliquities observed for stars at temperatures below the Kraft break [1]}, [2]}, [3]}, which may result from tidal damping [4]}, is not immediately evident at longer orbital periods, as shown in Figure REF .
